SLIM is a large area experiment (440m2) installed at the Chacaltaya cosmic ray laboratory since 2001, and about 100m2 at Koksil, Himalaya, since 2003. It is devoted to the search for intermediate mass magnetic monopoles (107–1013 GeV/c2) and nuclearites in the cosmic radiation using stacks of CR-39 and Makrofol nuclear track detectors. In four years of operation it will reach a sensitivity to a flux of about 10−15 cm−2 s−1 sr−1. We present the results of the calibration of CR-39 and Makrofol and the analysis of a first sample of the exposed detector.

Search for intermediate mass magnetic monopoles and nuclearites with the SLIM experiment / S. Cecchini; T. Chiarusi; D. Di Ferdinando;M. Cozzi;M. Frutti; G. Giacomelli; A. Kumar; S. Manzoor; J. McDonald; E. Medinaceli; J. Nogales ; L. Patrizii; J. Pinfold;V. Popa; I.E. Qureshi; O. Saavedra; G. Sher; M.I. Shahzad; M. Spurio; R. Ticona ;V. Togo;A.Velarde. - In: RADIATION MEASUREMENTS. - ISSN 1350-4487. - STAMPA. - 40:(2005), pp. 405-409. [10.1016/j.radmeas.2005.01.008]

Search for intermediate mass magnetic monopoles and nuclearites with the SLIM experiment

CECCHINI, STEFANO;CHIARUSI, TOMMASO;COZZI, MICHELA;GIACOMELLI, GIORGIO MARIA;MEDINACELI VILLEGAS, EDUARDO;PATRIZII, LAURA;POPA, VLAD;SPURIO, MAURIZIO;
2005

Abstract

SLIM is a large area experiment (440m2) installed at the Chacaltaya cosmic ray laboratory since 2001, and about 100m2 at Koksil, Himalaya, since 2003. It is devoted to the search for intermediate mass magnetic monopoles (107–1013 GeV/c2) and nuclearites in the cosmic radiation using stacks of CR-39 and Makrofol nuclear track detectors. In four years of operation it will reach a sensitivity to a flux of about 10−15 cm−2 s−1 sr−1. We present the results of the calibration of CR-39 and Makrofol and the analysis of a first sample of the exposed detector.
2005
Search for intermediate mass magnetic monopoles and nuclearites with the SLIM experiment / S. Cecchini; T. Chiarusi; D. Di Ferdinando;M. Cozzi;M. Frutti; G. Giacomelli; A. Kumar; S. Manzoor; J. McDonald; E. Medinaceli; J. Nogales ; L. Patrizii; J. Pinfold;V. Popa; I.E. Qureshi; O. Saavedra; G. Sher; M.I. Shahzad; M. Spurio; R. Ticona ;V. Togo;A.Velarde. - In: RADIATION MEASUREMENTS. - ISSN 1350-4487. - STAMPA. - 40:(2005), pp. 405-409. [10.1016/j.radmeas.2005.01.008]
S. Cecchini; T. Chiarusi; D. Di Ferdinando;M. Cozzi;M. Frutti; G. Giacomelli; A. Kumar; S. Manzoor; J. McDonald; E. Medinaceli; J. Nogales ; L. Patrizii; J. Pinfold;V. Popa; I.E. Qureshi; O. Saavedra; G. Sher; M.I. Shahzad; M. Spurio; R. Ticona ;V. Togo;A.Velarde
File in questo prodotto:
Eventuali allegati, non sono esposti

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/126406
 Attenzione

Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo

Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 16
  • ???jsp.display-item.citation.isi??? 14
social impact